A low level of extragalactic background light as revealed by γ-rays from blazars

Nature

Volumn 440, Issue 7087, 2006, Pages 1018-1021

  Aharonian, F ^a   Akhperjanian, A G ^b   Bazer Bachi, A R ^c   Beilicke, M ^d   Benbow, W ^a   Berge, D ^a   Bernlohr K ^a,e   Boisson, C ^c   Bolz, O ^a   Borrel, V ^c   Braun, I ^a   Breitling, F ^e   Brown, A M ^f   Chadwick, P M ^f   Chounet, L M ^g   Cornils, R ^d   Costamante, L ^a,h   Degrange, B ^g   Dickinson, H J ^f   Djannati Atai A ⁱ   Drury, L O'C ^j   Dubus, G ^g   Emmanoulopoulos, D ^k   Espigat, P ⁱ   Feinstein, F ^l   Fontaine, G ^g   Fuchs, Y ^c   Funk, S ^a   Gallant, Y A ^l   Giebels, B ^g   Gillessen, S ^a   Glicenstein, J F ^m   Goret, P ^m   Hadjichristidis, C ^f   Hauser, D ^a   Hauser, M ^k   Heinzelmann, G ^d   Henri, G ^c   Hermann, G ^a   Hinton, J A ^a   Hofmann, W ^a   Holleran, M ⁿ   Horns, D ^a   Jacholkowska, A ^l   De Jager, O C ⁿ   Khelifi B ^a   Klages, S ^a   Komin, Nu ^e   Konopelko, A ^e   Latham, I J ^f   Le Gallou, R ^f   Lemiere A ⁱ   Lemoine Goumard, M ^g   Leroy, N ^g   Lohse, T ^e   Martin, J M ^c   Martineau Huynh, O ^o   Marcowith, A ^c   Masterson, C ^a,h   McComb, T J L ^f   De Naurois, M ^o   Nolan, S J ^f   Noutsos, A ^f   Orford, K J ^f   Osborne, J L ^f   Ouchrif, M ^h,o   Panter, M ^a   Pelletier, G ^c   Pita, S ⁱ   Puhlhofer G ^k   Punch, M ⁱ   Raubenheimer, B C ⁿ   Raue, M ^d   Raux, J ^o   Rayner, S M ^f   Reimer, A ^p   Reimer, O ^p   Ripken, J ^d   Rob, L ^q   Rolland, L ^o   Rowell, G ^a   Sahakian, V ^b   Sauge L ^c   Schlenker, S ^e   Schlickeiser, R ^p   Schuster, C ^p   Schwanke, U ^e   Siewert, M ^p   Sol, H ^c   Spangler, D ^f   Steenkamp, R ^r   Stegmann, C ^e   Tavernet, J P ^o   Terrier, R ⁱ   Theoret C G ⁱ   Tluczykont, M ^g,h   Van Eldik, C ^a   Vasileiadis, G ^l   Venter, C ⁿ   Vincent, P ⁿ   Volk H J ^a   Wagner, S J ^k   more..

^a MAX PLANCK INSTITUT FÜR KERNPHYSIK   (Germany)

^b YEREVAN PHYSICS INSTITUTE   (Armenia)

^c CNRS   (France)

^d UNIVERSITY OF HAMBURG   (Germany)

^e HUMBOLDT UNIVERSITY   (Germany)

^f DURHAM UNIVERSITY   (United Kingdom)

^g ECOLE POLYTECHNIQUE   (France)

^h European Associated Laboratory for Gamma Ray Astronomy   (Germany)

ⁱ UNIVERSITÉ PARIS DIDEROT   (France)

^j DUBLIN INSTITUTE FOR ADVANCED STUDIES   (Ireland)

^k UNIVERSITÄT HEIDELBERG   (Germany)

^l UNIVERSITÉ MONTPELLIER II   (France)

^m CEA SACLAY   (France)

ⁿ NORTH WEST UNIVERSITY   (South Africa)

^o UNIVERSITÉ PARIS DIDEROT   (France)

^p RUHR UNIVERSITY BOCHUM   (Germany)

^q CHARLES UNIVERSITY   (Czech Republic)

^r UNIVERSITY OF NAMIBIA   (Namibia)

more..

Author keywords

[No Author keywords available]

Indexed keywords

GAMMA RAYS; LIGHT ABSORPTION; LIGHT EMISSION; LIGHT SOURCES;

EXTRAGALACTIC BACKGROUND LIGHT; EXTRAGALACTIC OBJECTS; FOREGROUND EMISSION; ZODIACAL LIGHT;

GALAXIES;

ASTRONOMY; EXTRATERRESTRIAL MATTER; GAMMA RAY RADIATION; INFRARED RADIATION; LIGHT; SOLAR SYSTEM;

ARTICLE; COSMOS; GAMMA RADIATION; LIGHT; MEASUREMENT; PHOTON; PRIORITY JOURNAL; SPACE; SPECTRAL SENSITIVITY; WAVEFORM;

EID: 33646197412     PISSN: 00280836     EISSN: 14764687     Source Type: Journal    
DOI: 10.1038/nature04680     Document Type: Article

References (30)

1. Hauser, M. G. & Dwek, E. The Cosmic Infrared Background: measurements and implications. Annu. Rev. Astron. Astrophys. 39, 249-307 (2001).
2. Nikishov, A. I. Absorption of high-energy photons in the universe. Sov. Phys. JETP 14, 393-394 (1962).
3. Gould, R. J. & Schreder, G. P. Opacity of the Universe to high-energy photons. Phys. Rev. Lett. 16, 252-254 (1966).
4. Jelley, J. V. High-energy gamma-ray absorption in space by a 3.5°K microwave field. Phys. Rev. Lett. 16, 479-481 (1966).
5. Stecker, F. W., De Jager, O. C. & Salamon, M. H. TeV gamma rays from 3C 279 - A possible probe of origin and intergalactic infrared radiation fields. Astrophys. J. Lett. 390, 49-52 (1992).
6. Aharonian, F. A. TeV blazars and the cosmic infrared background radiation. Invited, Rapporteur, and Highlight Papers of the Proc. 27th ICRC (Hamburg) (ed. Schlickeiser, R.) 250-262 (Copernicus Gesellschaft, Katlenburg-Lindau, 2001); preprint at 〈http://arXiV.org/astro-ph/0112314〉 (2001).
7. Costamante, L. & Ghisellini, G. TeV candidate BL Lac objects. Astron. Astrophys. 384, 56-71 (2002).
8. Madau, P. & Pozzetti, L. Deep galaxy counts, extragalactic background light and the stellar baryon budget. Mon. Not. R. Astron. Soc. 312L, 9-15 (2000).
9. Santos, M. R., Bromm, V. & Kamionkowski, M. The contribution of the first stars to the cosmic infrared background. Mon. Not. R. Astron. Soc. 336, 1082-1092 (2002).
10. Aharonian, F. A. et al. H.E.S.S. observations of PKS 2155-304. Astron. Astrophys. 430, 865-875 (2005).
11. Aharonian, F. A. et al. Observations of H1426+428 with HEGRA. Observations in 2002 and reanalysis of 1999 and 2000 data. Astron. Astrophys. 403, 523-528 (2003).
12. Primack, J. R., Somerville, R. S., Bullock, J. S. & Devriendt, J. E. G. Probing Galaxy formation with high-energy gamma rays. AIP Conf. Proc. 558, 463-478 (2001).
13. Dwek, E. & Krennrich, F. Simultaneous constraints on the spectrum of the extragalactic background light and the intrinsic TeV spectra of Mkn 421, Mkn 501, and H1426+428. Astrophys. J. 618, 657-674 (2005).
14. Dwek, E. & Arendt, R. G. A tentative detection of the cosmic infrared background at 3.5 μm from COBE/DIRBE observations. Astrophys. J. Lett. 508, 9-12 (1998).
15. Wright, E. L. DIRBE minus 2MASS: confirming the cosmic infrared background at 2.2 microns. Astrophys. J. 553, 538-544 (2001).
16. Matsumoto, T. et al. Infrared telescope in space observations of the near-infrared extragalactic background light. Astrophys. J. 626, 31-43 (2005).
17. Cambresy, L., Reach, W. T., Beichman, C. A. & Jarrett, T. H. The cosmic infrared background at 1.25 and 2.2 microns using DIRBE and 2MASS: A contribution not due to galaxies? Astrophys. J. 555, 563-571 (2001).
18. Kashlinsky, A. Cosmic infrared background and early galaxy evolution. Phys. Rep. 409, 361-438 (2005).
19. Aharonian, F. et al. The time averaged TeV energy spectrum of MKN 501 of the extraordinary 1997 outburst as measured with the stereoscopic Cherenkov telescope system of HEGRA. Astron. Astrophys. 349, 11-28 (1999).
20. Krennrich, F. et al. Discovery of spectral variability of Markarian 421 at TeV energies. Astrophys. J. Lett. 575, 9-13 (2002).
21. Djannati-Atai, A. et al. Very high energy gamma-ray spectral properties of MKN 501 from CAT Cherenkov telescope observations in 1997. Astron. Astrophys. 350, 17-24 (1999).
22. Malkov, M. A. & Drury, L. O'C. Nonlinear theory of diffusive acceleration of particles by shock waves. Rep. Prog. Phys. 64, 429-481 (2001).
23. Primack, J. R., Bullock, J. S. & Somerville, R. S. Observational gamma-ray cosmology. AIP Conf. Proc. 745, 23-33 (2005).
24. Madau, P. & Silk, J. Population III and the near-infrared background excess. Mon. Not. R. Astron. Soc. 359L, 37-41 (2005).
25. Dwek, E., Arendt, R. G. & Krennrich, F. The near infrared background: interplanetary dust or primordial stars? Astrophys. J. 635, 784-794 (2005).
26. Bernstein, R. A., Freedman, W. L. & Madore, B. F. The first detections of the extragalactic background light at 3000, 5500, and 8000 Å. I. Results. Astrophys. J. 571, 56-84 (2002).
27. Protheroe, R. J. & Meyer, H. An infrared background-TeV gamma-ray crisis? Phys. Lett. B 493, 1-6 (2000).
28. Fazio, G. G. et al. Number counts at 3 μm < λ < 10 μm from the Spitzer Space Telescope. Astrophys. J. Suppl. 154, 39-43 (2004).
29. Totani, T. et al. Diffuse extragalactic background light versus deep galaxy counts in the Subaru deep field: Missing light in the Universe? Astrophys. J. 550L, 137-141 (2001).
30. Mattila, K. Has the optical extragalactic background light been detected? Astrophys. J. 591, 119-124 (2003).